activity
20182025
most citedReviewing the frequency and central depletion of Ultra-Diffuse Galaxies in galaxy clusters from the KIWICS survey

47 citations · 115 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.IM2025

Unlocking the physics of dwarf galaxies in the 2040s: The case for a next-generation wide-field spectroscopic facility with fibres and IFUs

Crescenzo Tortora, Daniela Carollo, Leslie Hunt +25

Dwarf galaxies () are the most numerous galaxies in the Universe and critical probes of dark matter, baryonic feedback, and galaxy formation. D…

astro-ph.GA2025★ 18 cited

The galaxy-halo connection of disc galaxies over six orders of magnitude in stellar mass

Pavel E. Mancera Piña, Justin I. Read, Stacy Kim +5

(Abridged) The relations between stellar (), gas (), baryonic (), and dark matter halo mass () provide unique cons…

astro-ph.GA2025★ 6 cited

MIGHTEE-HI: The direct detection of neutral hydrogen in galaxies at

Matt J. Jarvis, Madalina N. Tudorache, I. Heywood +18

Atomic hydrogen constitutes the gas reservoir from which molecular gas and star formation in galaxies emerges. However, the weakness of the line means it has been difficult to dire…

astro-ph.GA2025★ 11 cited

Ages and metallicities of quiescent galaxies: confronting broadband () colours with stellar absorption lines

Chloe M. Cheng, Mariska Kriek, Aliza G. Beverage +9

For decades, studying quiescent galaxies beyond has been challenging due to the reliance on photometric spectral energy distributions, which are highly susceptible to dege…

astro-ph.GA2025★ 10 cited

Photometric vs dynamical stellar masses and their impact on scaling relations in nearby disc galaxies

A. Marasco, S. M. Fall, E. M. Di Teodoro +1

The study of scaling relations of disc galaxies and their evolution across cosmic time requires accurate estimates of galaxy stellar masses over broad redshift ranges. Wh…

astro-ph.GA2025★ 7 cited

MIGHTEE-HI: The radial acceleration relation with resolved stellar mass measurements

Andreea A. Vărăşteanu, Matt J. Jarvis, Anastasia A. Ponomareva +8

The radial acceleration relation (RAR) is a fundamental relation linking baryonic and dark matter in galaxies by relating the observed acceleration derived from dynamics to the one…

astro-ph.GA2025★ 2 cited

The angular momentum -- mass relation of local disc galaxies

Nikki N. Geesink, Pavel E. Mancera Piña, Claudia del P. Lagos +1

We present an analysis of the molecular specific angular momentum-mass () relation using a sample of 51 nearby disc galaxies from the PHANGS-ALMA survey with deep,…

astro-ph.GA2024★ 7 cited

WALLABY Pilot Survey: Gas-Rich Galaxy Scaling Relations from Marginally-Resolved Kinematic Models

N. Deg, N. Arora, K. Spekkens +21

We present the first set of galaxy scaling relations derived from kinematic models of the Widefield ASKAP L-band Legacy All-sky Blind surveY (WALLABY) pilot phase observations. Com…

astro-ph.GA2024★ 7 cited

Photometry and kinematics of dwarf galaxies from the Apertif HI survey

Barbara Šiljeg, Elizabeth A. K. Adams, Filippo Fraternali +13

Context. Understanding the dwarf galaxy population in low density environments is crucial for testing the LCDM cosmological model. The increase in diversity towards low mass galaxi…

astro-ph.GA2024

A 3D view on the local gravitational instability of cold gas discs in star-forming galaxies at

C. Bacchini, C. Nipoti, G. Iorio +6

Local gravitational instability (LGI) is considered crucial for regulating star formation and gas turbulence in galaxy discs, especially at high redshift. Instability criteria usua…

astro-ph.GA2018★ 47 cited

Reviewing the frequency and central depletion of Ultra-Diffuse Galaxies in galaxy clusters from the KIWICS survey

Pavel E. Mancera Piña, Reynier F. Peletier, J. A. L. Aguerri +3

The number of Ultra-Diffuse Galaxies (UDGs) in clusters is of significant importance to constrain models of their formation and evolution. Furthermore, their distribution inside cl…